Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-26T13:33:05.414Z Has data issue: false hasContentIssue false
  • English
  • Français

Lyman Lines in Prominences and Filaments: NLTE Modelling Strategies

Published online by Cambridge University Press:  12 April 2016

P. Heinzel
P. Heinzel*
Affiliation:
Astronomical Institute, Academy of Sciences of the Czech Republic CZ–25165 Ondřejov, Czech Republic

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We briefly summarize the most important aspects of NLTE formation of hydrogen Lyman lines in prominences and filaments. A modified MALI code of Heinzel (1995) is described and its applicability to the interpretation of SOHO/SUMER data is discussed.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 188 - 189
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Gorshkov, A.B. 1997, in Science with Themis, (eds.) Mein, N. and SahalBréchot, S., Observatoire de Paris, p. 273 Google Scholar
Gouttebroze, et al. 1978, ApJ, 225, 655 Google Scholar
Gouttebroze, P., Heinzel, P. and Vial, J.-C. 1993, A&AS, 99, 513 Google Scholar
Heinzel, P. 1995, A&A, 299, 563 Google Scholar
Heinzel, P., Schmieder, B. and Vial, J.-C. 1997, in The Corona and Solar Wind Near Minimum Activity, ESA-SP 404, p. 427 Google Scholar
Hubený, I., Hummer, D.G. and Lanz, T. 1994, A&A, 282, 151 Google Scholar
Mein, N. et al. 1996, A&A, 309, 275 Google Scholar
Paletou, F. 1995, A&A, 302, 587 Google Scholar
Rybicki, G.B. and Hummer, D.G. 1991, A&A, 245, 171 Google Scholar